Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..150..347b&link_type=abstract
Solar Physics, vol. 150, no. 1-2, p. 347-357
Astronomy and Astrophysics
Astronomy
23
Hysteresis, Phase Shift, Radio Astronomy, Solar Activity, Solar Corona, Solar Cycles, Solar Magnetic Field, Solar Radio Emission, Sunspots, Time Lag, Ultraviolet Astronomy, Ultraviolet Emission, Variations, Electron Energy, Flux (Rate), Flux Density, Lissajous Figures, Lyman Alpha Radiation, Nimbus 7 Satellite, Noaa 9 Satellite, Solar Electrons, Time Series Analysis
Scientific paper
We show that smoothed time series of 7 indices of solar activity exhibit significant solar cycle dependent differences in their relative variations during the past 20 years. In some cases these observed hysteresis patterns start to repeat over more than one solar cycle, giving evidence that this is a normal feature of solar variability. Among the indices we study, we find that the hysteresis effects are approximately simple phase shifts, and we quantify these phase shifts in terms of lag times behind the leading index, the International Sunspot Number. Our measured lag times range from less than one month to greater than four months and can be much larger than lag times estimated from short-term variations of these same activity indices during the emergence and decay of major active regions. We argue that hysteresis represents a real delay in the onset and decline of solar activity and is an important clue in the search for physical processes responsible for changing solar emission at various wavelengths.
Bachmann Kurt T.
White Oran Richard
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